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Multiple Simultaneous Gamma-Ray Emission Sites in 3c 84

J. A. Hodgson, S. S. Lee, B. Rani, J. C. Algaba

Труды ИПА РАН, вып. 41, 69–72 (2017)

Ключевые слова: VLBI, γ-rays

Аннотация

The mis-aligned active galactic nuclei (AGN), 3C 84, has been observed approximately monthly at four frequencies simultaneously (22–129 GHz) on the Korean VLBI Network (KVN) since 2013 as part of the interferometric monitoring of γ-ray bright AGN (iMOGABA) program. 3C 84 is known to have to sites of bright radio emission, with the first thought to be near the central super-massive black hole and the second in a slowly moving emission feature, several milliarcseconds south of the core. Analysis of this data suggests that the highly variable γ-ray emission originates near the SMBH and the slowly rising γ-ray emission originates in the slow moving feature.

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J. A. Hodgson, S. S. Lee, B. Rani, J. C. Algaba. Multiple Simultaneous Gamma-Ray Emission Sites in 3c 84 // Труды ИПА РАН. — 2017. — Вып. 41. — С. 69–72.

@article{hodgson2017,
  abstract = {The mis-aligned active galactic nuclei (AGN), 3C 84, has been observed approximately monthly at four frequencies simultaneously (22–129 GHz) on the Korean VLBI Network (KVN) since 2013 as part of the interferometric monitoring of γ-ray bright AGN (iMOGABA) program. 3C 84 is known to have to sites of bright radio emission, with the first thought to be near the central super-massive black hole and the second in a slowly moving emission feature, several milliarcseconds south of the core. Analysis of this data suggests that the highly variable γ-ray emission originates near the SMBH and the slowly rising γ-ray emission originates in the slow moving feature.},
  author = {J.~A. Hodgson and S.~S. Lee and B. Rani and J.~C. Algaba},
  issue = {41},
  journal = {Труды ИПА РАН},
  keyword = {VLBI, γ-rays},
  pages = {69--72},
  title = {Multiple Simultaneous Gamma-Ray Emission Sites in 3c 84},
  url = {http://iaaras.ru/library/paper/1707/},
  year = {2017}
}

TY  - JOUR
TI  - Multiple Simultaneous Gamma-Ray Emission Sites in 3c 84
AU  - Hodgson, J. A.
AU  - Lee, S. S.
AU  - Rani, B.
AU  - Algaba, J. C.
PY  - 2017
T2  - Труды ИПА РАН
IS  - 41
SP  - 69
AB  - The mis-aligned active galactic nuclei (AGN), 3C 84, has been
observed approximately monthly at four frequencies simultaneously
(22–129 GHz) on the Korean VLBI Network (KVN) since 2013 as part of
the interferometric monitoring of γ-ray bright AGN (iMOGABA) program.
3C 84 is known to have to sites of bright radio emission, with the
first thought to be near the central super-massive black hole and the
second in a slowly moving emission feature, several milliarcseconds
south of the core. Analysis of this data suggests that the highly
variable γ-ray emission originates near the SMBH and the slowly
rising γ-ray emission originates in the slow moving feature.
UR  - http://iaaras.ru/library/paper/1707/
ER  -